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Star profile

72 Cygni

3D likeness based on its real data · class K · ~4,200 K

What is 72 Cygni

72 Cygni burns some 232 light-years away as an orange K-type giant within Cygnus, the swan flying along the summer Milky Way. Its outer envelope, swollen and cooled after exhausting core hydrogen, gives it that characteristic amber tone. The constellation is crossed by the Great Rift of galactic dust, against which this star stands out like a warm ember. Its light departed around 1793.

Where it is and when to see it

72 Cygni lies in the northern celestial hemisphere. It is visible to the naked eye under a dark sky. Its best month of the year is September, when it culminates around midnight.

  • From London it never sets and culminates about 77° up.
  • From New York it culminates about 88° above the horizon.
  • From Sydney it culminates about 18° above the horizon.

It can be seen from anywhere north of 51° S.

It ranks no. 36 in brightness among the 137 stars of Cygnus in our catalogue. To find it, start from Deneb, the brightest: it lies about 12° away (a fist at arm's length covers about 10°).

The light you see today left it about 230 years ago.

Find it on the sky map

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Leave your signature on 72 Cygni

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A public signature from a real person. The chosen name is a symbolic denomination within Stelvia, with no official standing or IAU recognition: the sky is not for sale and belongs to no one.

Astronomical data for 72 Cygni

Constellation
Cygnus
Apparent magnitude
4.87
Distance
231.5 light years
Coordinates (J2000)
RA 323.694° · Dec 38.534°
Catalogue
HIP 106551 · HD 205512

A symbolic commemorative gift: neither the signature nor the chosen name implies ownership of the star or recognition by the IAU.

Other stars in Cygnus

Cygnus has 137 stars in Stelvia's catalogue. Here are a few of them.

See all 137 stars in Cygnus